Stability Of Planetary Orbits
Stability of Planetary Orbits is a theoretical construct in celestial mechanics that characterizes the long-term persistence of planetary trajectories within bounded deviations from nominal paths under perturbative gravitational influences.
341
Publications
23K
Citations
729
Authors
307
Institutions
Publications per year
2017–2026
53
Parents
341
Shrinking Binary and Planetary Orbits by Kozai Cycles with Tidal Friction
The Astrophysical Journal · 2007 · 1.4K citations · Full text
Natural Sciences, Astronomy, Physics +17
Long-Term Stability of Planets in Binary Systems
The Astronomical Journal · 1999 · 863 citations · Full text
Natural Sciences, Astronomy, Physics +16
Dynamics of Systems of Two Close Planets
Brett Gladman · Icarus · 1993 · 639 citations
Natural Sciences, Astronomy, Physics +16
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307
University of Vienna
Vienna, Austria
18 h-index
45 publications
2.3K citations

Ames Research Center
Mountain View, United States
17 h-index
68 publications
9.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
15 h-index
45 publications
6.5K citations

Centre National de la Recherche Scientifique
Paris, France
15 h-index
44 publications
1.6K citations
The University of Texas at Arlington
Arlington, United States
13 h-index
33 publications
1.5K citations
Observatoire de la Côte d’Azur
Nice, France
13 h-index
18 publications
1.3K citations
University of California, Santa Cruz
Santa Cruz, United States
13 h-index
17 publications
1.6K citations
University of Michigan
Ann Arbor, United States
13 h-index
22 publications
1.4K citations
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ApJ · 56 publications · 6.4K citations
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51 publications · 2.1K citations
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AJ · 37 publications · 3.7K citations
27
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31 publications · 1.3K citations
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26 publications · 946 citations
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